Determining the strange and antistrange quark distributions of the nucleon

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. Zeller G P et al (NuTeV collaboration). Phys. Rev. Lett.,2002, 88: 0918022. Airapetian A et al (HERMES collaboration). Phys. Lett.B, 2008, 666: 4463. Bazarko A O et al (CCFR collaboration). Z. Phys. C, 1995,65: 1894. Goncharov M et al (NuTeV collaboration). Phys. Rev. D,2001, 64: 1120065. For recent reviews, see e.g., Kumano S. Phys. Rep., 1998,303: 103; Speth J, Thomas A W. Adv. Nucl. Phys., 1998,24: 836. Signal A I, Thomas A W. Phys. Lett. B, 1987, 191: 2057. CAO F G, Signal A I. Phys. Rev. D, 1999, 60: 0740218. Thomas A W. Phys. Lett., 1983, 126B: 979. Holtmann H, Szczurek A, Speth J. Nucl. Phys. A, 1996,569: 63110. CAO F G, Signal A I. Eur. Phys. J., 2001, C 21: 10511. CAO F G, Signal A I. Phys. Lett. B, 2003, 559: 22912. Bissey F, CAO F G, Signal A I. Phys. Rev. D, 2006, 73:07400813. CHEN H, CAO F G, Signal A I. in preparation14. Martin A D, Stirling W J, Thorne R S, Watt G. arXiv:0901.0002 [hep-ph]15. Nadolsky P M et al. Phys. Rev. D, 2008, 78: 013004 arXi:0802.00007 [hep-ph]16. LAI H L et al. J. High Energy Phys., 2007, 0704: 08917. Tung W K et al. J. High Energy Phys., 2007, 02: 053